KLENOT - Klet Observatory Near Earth and Other Unusual Objects Observations Team and Telescope

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00070327%3A_____%2F02%3A00006656" target="_blank" >RIV/00070327:_____/02:00006656 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/00070327:_____/02:00014362

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

KLENOT - Klet Observatory Near Earth and Other Unusual Objects Observations Team and Telescope

Popis výsledku v původním jazyce

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects (NEOs), distant objects and comets. The improved effort of the large NEO surveys has resulted in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies, first in discovery opposition and then during next apparitions. Moreover, recently added automatic impact monitoring systems require additional accurate astrometry of potential future Earth impactors (Virtual Impactors) to remove, or to confirm, possible impact solutions. Many of these targets are objects fainter than magnitude mV=20.0m. Considering both these urgent need of astrometric follow-up and our results and experience in minor planet and comet CCD astrometry, done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The KLENO

Název v anglickém jazyce

KLENOT - Klet Observatory Near Earth and Other Unusual Objects Observations Team and Telescope

Popis výsledku anglicky

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects (NEOs), distant objects and comets. The improved effort of the large NEO surveys has resulted in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies, first in discovery opposition and then during next apparitions. Moreover, recently added automatic impact monitoring systems require additional accurate astrometry of potential future Earth impactors (Virtual Impactors) to remove, or to confirm, possible impact solutions. Many of these targets are objects fainter than magnitude mV=20.0m. Considering both these urgent need of astrometric follow-up and our results and experience in minor planet and comet CCD astrometry, done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The KLENO

Druh

D - Stať ve sborníku

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

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Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2002

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Proceedings of the Conference Asteroids, Comets, Meteors 2002

ISBN

92-9092-810-7

ISSN

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e-ISSN

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Počet stran výsledku

4

Strana od-do

793-796

Název nakladatele

ESA-ESTEC, NL

Místo vydání

Noordwijk, NL

Místo konání akce

Berlin, Germany

Datum konání akce

1. 1. 2002

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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